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DENIS J104731.1-181558
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Star DENIS J104731.1-181558

Brown dwarf DENIS J104731.1-181558 is located 92 light years away from the Sun. It is a single star of spectral class L0.3V, that has typically about 4 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
92 light years

DENIS J104731.1-181558

Spectral class: L0.3V

Location +

Ascension iconRight ascension: 10h 47m 30.655s
Declination iconDeclination: -18° 15' 56.712'' (equatorial region)
Parallax iconParallax: 35.589
Distance iconSun distance: 91.646 ly | 28.1 pc
Star position
The position of a star tells us where it appears in the sky, similar to how we use coordinates like latitude and longitude on Earth. In astronomy, the three main coordinates are right ascension, declination and distance. .. icon More about Star position in StellarGuide

Basic characteristic

icon weight
Mass: 8 % M Sun
| 83.8 M Jupiter
 (estimate)
+
Star mass
The estimated mass of the star DENIS J104731.1-181558 is about 8 % of the Sun's mass, or approximately 83.8 Jupiter masses.

The mass of a star is the total amount of matter it contains. It is one of the most important properties of a star, as it determines almost everything about how the star lives, changes, and dies. In astronomy, star mass is usually measured in solar masses (M☉) — where 1 solar mass is equal to the mass of our Sun... icon More about Star mass in StellarGuide
temperature iconTemperature: 2300 K
 (estimate)
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Star temperature
Surface temperature of DENIS J104731.1-181558 is estimated to be 2250 K, which is 40 % of the temperature on the surface of the Sun.

The temperature of a star refers to the temperature at its surface, also called the photosphere. It is measured in kelvins (K), the standard unit for temperature in astronomy. A star’s temperature tells us a lot about its physical properties and where it stands in its evolutionary stage... icon More about Star temperature in StellarGuide

Photometry

Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).
5
10
15
20
25
30
35
K
2.1
H
1.6
J
1.2
Grp
0.8
I
0.8
G
0.6
V
0.5
Gbp
0.5
B
0.4
U
0.3
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DENIS J104731.1-181558 system structure

DENIS J104731.1-181558

More about DENIS J104731.1-181558

       DENIS J104731.1-181558 can be found in southern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope. 
Other designations of this star
Gaia DR3 3555963059703156224
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External sources
simbad icon
Simbad database (DENIS J104731.1-181558)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia DR3 3555963059703156224)
Archive from the Gaia mission

Frequently Asked Questions

How far is the DENIS J104731.1-181558 system from the Sun?

The DENIS J104731.1-181558 system is 92 light years or 28.1 parsecs from the Sun.

What galaxy is the DENIS J104731.1-181558 star in?

The DENIS J104731.1-181558 is in the Milky Way galaxy just like the Sun.

How many stars are in the DENIS J104731.1-181558 system?

The DENIS J104731.1-181558 is a single star, there are no other known stars in the system.

What type of star is the DENIS J104731.1-181558?

The star DENIS J104731.1-181558 is a Brown dwarf star.

What temperature is the DENIS J104731.1-181558?

The primary in the DENIS J104731.1-181558 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
Class of stars Brown dwarf
Brown dwarfs are not really stars, because there is no thermonuclear fusion in their core. These objects are smaller and cooler than stars, but too massive to be considered planets.
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stellar brief logoStellar Brief

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3. 11. 2026
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TOI-2298 b is about three times Earth’s size and circles its orange dwarf star inside the star’s conservative habitable zone, but uncertain orbits can make such labels misleading. New studies also examine the dust around HD 100546, a possible giant planet around HD 156295, a changing planetary orbit, and how computer models interpret exoplanet atmospheres.
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